130,761 research outputs found

    Aspect-ratio dependence of the transition to the ultimate state of turbulent Rayleigh-Bénard convection

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    We report on measurements of the ultimate-state transition in turbulent Rayleigh-B\'enard convection obtained in a large facility known as the ``Uboot of G\"ottingen" and using pressurized sulfur hexafluoride as the convecting fluid. We found that the transition occurs over a range of RaRa which becomes more narrow as Γ\Gamma increases, ranging from Ra1Ra_1^* which is at most weakly dependent on Γ\Gamma and close to 101310^{13} to Ra2Ra_2^* which varies from about 2×10152\times 10^{15} for Γ=0.33\Gamma = 0.33 to about 7×10137\times 10^{13} for Γ=1.00\Gamma = 1.00

    The Göttingen rotating turbulent Rayleigh-Bénard convection facility

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    Thermally driven turbulent convection under the influence of global rotation is ubiquitous in nature. Well known examples are the outer convective shell of our Sun and the outer liquid core of the Earth. Trying to understand the underlying dynamics of such flows is highly challenging, not only because of the enormous range in length- and time-scales that are involved with these geo/astrophysical cases and the complex interaction of hydrodynamics with electromagnetism, but also because direct measurements on these systems are most often impossible to carry out. We gain access to direct measurements by isolating part of the problem: We focus solely on the hydrodynamical aspects of turbulent convection by performing experiments in the lab and making comparisons with direct numerical simulations (DNS). The canonical system that we use to study such flows is Rayleigh-B\'enard convection (RBC), the flow between a warm bottom plate and cold top plate, in a fluid-filled upright cylindrical cell that is rotating around its geometrical axis. This presentation will focus on the newly constructed rotating RBC facility at the Max Planck Institute for Dynamics and Self-Organization (MPIDS) in G\"ottingen

    MeSH term explosion and author rank improve expert recommendations

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    Information overload is an often-cited phenomenon that reduces the productivity, efficiency and efficacy of scientists. One challenge for scientists is to find appropriate collaborators in their research. The literature describes various solutions to the problem of expertise location, but most current approaches do not appear to be very suitable for expert recommendations in biomedical research. In this study, we present the development and initial evaluation of a vector space model-based algorithm to calculate researcher similarity using four inputs: 1) MeSH terms of publications; 2) MeSH terms and author rank; 3) exploded MeSH terms; and 4) exploded MeSH terms and author rank. We developed and evaluated the algorithm using a data set of 17,525 authors and their 22,542 papers. On average, our algorithms correctly predicted 2.5 of the top 5/10 coauthors of individual scientists. Exploded MeSH and author rank outperformed all other algorithms in accuracy, followed closely by MeSH and author rank. Our results show that the accuracy of MeSH term-based matching can be enhanced with other metadata such as author rank

    Going Beyond Counting First Authors in Author Co-citation Analysis

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    The present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed

    Rayleigh-B\'enard convective motion of stratified fluids in the Earth's troposphere

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    Recently, Kaladze and Misra [Phys. Scr. 99 (2024) 085013] showed that the tropospheric stratified fluid flows may be unstable by the effects of the negative temperature gradient and the temperature-dependent density inhomogeneity arising from the thermal expansion. They also predicted that the modification in the Brunt-V\"ais\"al\"a frequency by the density inhomogeneity can lead to Rayleigh-B\'enard convective instability in the tropospheric unbounded layers. The purpose of the present work is to revisit the Rayleigh-B\'enard convective instability in more detail by considering both unbounded and bounded tropospheric layers. We show that the conditions for instability in these two cases significantly differ. The critical values of the Raleigh numbers and the expressions for the instability growth rates of thermal waves in the two cases are obtained and analyzed. In the case of the bounded region, we also derive the necessary boundary conditions and note that the vertical wave number is quantified, and the corresponding eigenvalue problem is well-set.Comment: 10 pages, 5 figure

    "Closing the R&D Gap, Evaluating the Sources of R&D Spending"

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    Both spending and tax policies have been implemented in the United States with the goal of stimulating private sector research and development (R&D). Karier questions whether current R&D policy, especially the research and experimentation tax credit, can contribute to closing the gap between nondefense expenditures on R&D in the United States and such expenditures in other countries, such as Japan and Germany. He also explores possible changes to our current R&D policy to make it more effective.

    Dynamics of large-scale structures and heat transfer in turbulent mixed convection

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    Low frequency oscillations have been observed in the heat transfer of mixed convection in a rectangular cavity with an aspect ratio of Γxz=1\Gamma_{\mathrm{xz}} = 1 and Γyz=5\Gamma_{\mathrm{yz}} = 5.~Mixed convective flow at Ra=2.4×108Ra = 2.4 \times 10^8, Re=1.0×104Re = 1.0 \times 10^{4}, Ar=3.3Ar = 3.3 and Pr0.7Pr \approx 0.7 has been studied to determine the nature of these oscillations. Therefore Particle Image Velocimetry (PIV) and temperature measurements have been performed under ambient and high pressure conditions. The PIV results have been analysed using Proper Orthogonal Decomposion (POD) to identify the characteristic frequencies of the coherent large-scale structures and their dynamics have been compared with the low frequency oscillations found in the heat transfer

    Evaporating Rayleigh-B\'enard convection: prediction of interface temperature and global heat transfer modulation

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    We propose an analytical model to estimate the interface temperature ΘΓ\Theta_{\Gamma} and the Nusselt number NuNu for an evaporating two-layer Rayleigh-B\'enard configuration in statistically stationary conditions. The model is based on three assumptions: (i) the Oberbeck-Boussinesq approximation can be applied to the liquid phase, while the gas thermophysical properties are generic functions of thermodynamic pressure, local temperature, and vapour composition, (ii) the Grossmann-Lohse theory for thermal convection can be applied to the liquid and gas layers separately, (iii) the vapour content in the gas can be taken as the mean value at the gas-liquid interface. We validate this setting using direct numerical simulations (DNS) in a parameter space composed of the Rayleigh number (106Ra10810^6\leq Ra\leq 10^8) and the temperature differential (0.05ε0.200.05\leq\varepsilon\leq 0.20), which modulates the variation of state variables in the gas layer. To better disentangle the variable property effects on ΘΓ\Theta_\Gamma and NuNu, simulations are performed in two conditions. First, we consider the case of uniform gas properties except for the gas density and gas-liquid diffusion coefficient. Second, we include the variation of specific heat capacity, dynamic viscosity, and thermal conductivity using realistic equations of state. Irrespective of the employed setting, the proposed model agrees very well with the numerical simulations over the entire range of RaεRa-\varepsilon investigated

    A. D. Fricke, author

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    Black and white photograph of author, A. D. Fricke
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